SN 2007bi: Difference between revisions
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{{Short description|Supernova in the constellation Virgo}} |
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{{no footnotes|date=April 2015}} |
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{{Supernova |
{{Supernova |
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| name = SN 2007bi |
| name = SN 2007bi |
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| caption = SN 2007bi |
| caption = SN 2007bi |
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| epoch = [[J2000.0]] |
| epoch = [[J2000.0]] |
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| type = [[Type Ic |
| type = [[Type Ib and Ic supernovae|type Ic]] |
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| SNRtype = |
| SNRtype = |
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| host = [[Anon J131920+0855]] |
| host = [[Anon J131920+0855]] |
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| constellation = |
| constellation = [[Virgo (constellation)|Virgo]] |
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| ra =13<sup>h</sup> 19<sup>m</sup> 20.19<sup>s</sup> |
| ra =13<sup>h</sup> 19<sup>m</sup> 20.19<sup>s</sup> |
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| dec = +08° 55' 44.3'' |
| dec = +08° 55' 44.3'' |
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| mag_v = |
| mag_v = |
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| distance = |
| distance = |
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| notes = |
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| notes = is located near the apparent host galaxy [[Anon J131920+0855]] |
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| names = SN 2007bi |
| names = SN 2007bi |
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| progenitor = |
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}} |
}} |
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'''SN 2007bi''' was an extremely energetic [[supernova]] discovered early in 2007 by the international [[Nearby Supernova Factory]] based at the U.S. Department of Energy's [[Lawrence Berkeley National Laboratory]]. The precursor star is estimated to have had 200 solar masses at the time of its formation and around 100 solar masses in its core when it went supernova. The explosion ejected more than 22 solar masses of silicon and other heavy elements into space during this supernova including more than 6 solar masses of radioactive nickel which caused the expanding gases to glow very brightly for many months. |
'''SN 2007bi''' was an extremely energetic [[supernova]] discovered early in 2007 by the international [[Nearby Supernova Factory]] based at the U.S. Department of Energy's [[Lawrence Berkeley National Laboratory]]. The precursor star is estimated to have had 200 solar masses at the time of its formation and around 100 solar masses in its core when it went supernova. The explosion ejected more than 22 solar masses of silicon and other heavy elements into space during this supernova including more than 6 solar masses of radioactive nickel which caused the expanding gases to glow very brightly for many months. |
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==References== |
==References== |
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=={{1243142}} |
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* [http://simbad.u-strasbg.fr/simbad/sim-id?Ident=sn+2007bi&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id SIMBAD data] |
* [http://simbad.u-strasbg.fr/simbad/sim-id?Ident=sn+2007bi&NbIdent=1&Radius=2&Radius.unit=arcmin&submit=submit+id SIMBAD data] |
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===Open Section=== |
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Change this section to not make this a stub. |
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===<big>fvrrrgbwdfthw</big> |
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# 1273794 |
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# 1525735 |
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==Further reading== |
==Further reading== |
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*{{Citation | |
*{{Citation |last1=Gal-Yam |first1=A. |last2=Mazzali |first2=P. |last3=Ofek |first3=E. O. |year=2009 |title=Supernova 2007bi as a pair-instability explosion |journal=[[Nature (journal)|Nature]] |volume=462 |issue=7273 |pages=624–627 |doi=10.1038/nature08579 |bibcode = 2009Natur.462..624G |arxiv = 1001.1156 |pmid=19956255|s2cid=4336232 |display-authors=etal}} |
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==External links== |
==External links== |
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* [https://sne.space/sne/SN2007bi/ Light curves and spectra] {{Webarchive|url=https://web.archive.org/web/20190810152016/https://sne.space/sne/SN2007bi/ |date=2019-08-10 }} on the [https://sne.space Open Supernova Catalog] {{Webarchive|url=https://web.archive.org/web/20160303230459/https://sne.space/ |date=2016-03-03 }} |
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* New Scientist, [http://www.newscientist.com/article/dn18228-death-of-rare-giant-star-sheds-light-on-cosmic-past.html "Death of rare giant star sheds light on cosmic past"] <!--, '''David Shiga''', ''18:00 02 December 2009'' (accessed 07-12-2009) --> |
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* |
* New Scientist, [https://www.newscientist.com/article/dn18228-death-of-rare-giant-star-sheds-light-on-cosmic-past.html "Death of rare giant star sheds light on cosmic past"] <!--, '''David Shiga''', ''18:00 02 December 2009'' (accessed 07-12-2009) --> |
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* |
* Science Daily, [https://www.sciencedaily.com/releases/2009/12/091202153939.htm "Superbright Supernova Is First of Its Kind"] <!--, ''5 December 2009'' (accessed 07-12-2009) --> |
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* Keck Observatory, [https://web.archive.org/web/20110720180302/http://keckobservatory.org/index.php/news/first_of_its_kind_superbright_supernova "First of its kind superbright supernova"] <!--, ''2009'' (accessed 07-12-2009) --> |
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* Nature, [http://www.weizmann.ac.il/home/galyam/PTF/SN2007bi.pdf "Full report submitted by scientists to the journal Nature"] <!--, ''2009'' (accessed 07-12-2009) --> |
* Nature, [http://www.weizmann.ac.il/home/galyam/PTF/SN2007bi.pdf "Full report submitted by scientists to the journal Nature"] <!--, ''2009'' (accessed 07-12-2009) --> |
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* Weizmann Institute, [http://www.weizmann.ac.il/home/galyam/SNF20070406-008.html "First hand description of the study"] <!--, ''2010'' (accessed 02-01-2010) --> |
* Weizmann Institute, [http://www.weizmann.ac.il/home/galyam/SNF20070406-008.html "First hand description of the study"] <!--, ''2010'' (accessed 02-01-2010) --> |
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{{Supernovae}} |
{{Supernovae}}{{Virgo}} |
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{{DEFAULTSORT:SN 2007bi}} |
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[[Category:Supernovae]] |
[[Category:Supernovae]] |
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[[Category:Astronomical objects discovered in 2007]] |
[[Category:Astronomical objects discovered in 2007|20070406]] |
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[[Category: |
[[Category:Virgo (constellation)]] |
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{{ |
{{var-star-stub}} |
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{{sky|13|19|20.19|+|08|55|44.3}} |
{{sky|13|19|20.19|+|08|55|44.3}} |
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[[fr:SN 2007bi]] |
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[[hu:SN 2007bi]] |
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[[pl:SN 2007bi]] |
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[[zh:SN 2007bi]] |
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Latest revision as of 13:02, 15 November 2024
 | This article includes a list of references, related reading, or external links, but its sources remain unclear because it lacks inline citations. (April 2015) |
| Event type | Supernova  |
|---|---|
| type Ic | |
| Date | by Nearby Supernova Factory USA |
| Constellation | Virgo |
| Right ascension | 13h 19m 20.19s |
| Declination | +08° 55' 44.3 |
| Epoch | J2000.0 |
| Galactic coordinates | 324.1496 +70.6427 |
| Host | Anon J131920+0855 |
| Other designations | SN 2007bi |
SN 2007bi was an extremely energetic supernova discovered early in 2007 by the international Nearby Supernova Factory based at the U.S. Department of Energy's Lawrence Berkeley National Laboratory. The precursor star is estimated to have had 200 solar masses at the time of its formation and around 100 solar masses in its core when it went supernova. The explosion ejected more than 22 solar masses of silicon and other heavy elements into space during this supernova including more than 6 solar masses of radioactive nickel which caused the expanding gases to glow very brightly for many months.
The supernova has been described as an unambiguous fit for the pair-instability supernova model.
References
[edit]Further reading
[edit]- Gal-Yam, A.; Mazzali, P.; Ofek, E. O.; et al. (2009), "Supernova 2007bi as a pair-instability explosion", Nature, 462 (7273): 624–627, arXiv:1001.1156, Bibcode:2009Natur.462..624G, doi:10.1038/nature08579, PMID 19956255, S2CID 4336232
External links
[edit]- Light curves and spectra Archived 2019-08-10 at the Wayback Machine on the Open Supernova Catalog Archived 2016-03-03 at the Wayback Machine
- New Scientist, "Death of rare giant star sheds light on cosmic past"
- Science Daily, "Superbright Supernova Is First of Its Kind"
- Keck Observatory, "First of its kind superbright supernova"
- Nature, "Full report submitted by scientists to the journal Nature"
- Weizmann Institute, "First hand description of the study"
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